HSC 1416

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0.53 UTI
0.31
CN
0.97
Cdens
0.75
CC3
0.31
Clit
1.0
Cdup
Radius (P>50% members) 2.0 [arcmin]
  • CN 0.31 Poorly populated
  • Cdens 0.97 Very dense
  • CC3 0.75 High quality
  • Clit 0.31 Poorly studied
  • Cdup 1.0 Unique

Overview

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HSC 1416 is a poorly populated, very dense object of high C3 quality. Its parallax locates it at a moderate distance, below the mid-plane, affected by moderate extinction. It is catalogued as a near-solar metallicity, intermediate-age cluster (see Parameters). It was recently reported in the literature.
Distant Moderate extinction Near-solar metallicity Intermediate age

Cavallo et al. (2024)
Gold sample.

Data

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Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC – 83.801 28.064 0.23 1.064 -0.234 33.887
Hu & Soubiran 2025 83.802 28.055 – – – –
Zhang et al. 2024 83.804 28.073 – – – –
Hunt & Reffert 2024 83.804 28.073 0.213 1.076 -0.277 21.924
Cavallo et al. 2024 83.802 28.055 0.213 – – –
Hunt & Reffert 2023 83.804 28.073 0.213 1.076 -0.277 21.924

💡 Note: The UCC values are estimated from its identified members.

Reference Year Dist [kpc] Av [mag] DAv [mag] Age [Myr] [Fe/H] [dex] Mass [Msun] Bfr BSS
Hu & Soubiran 2025 – – – – -0.490* – – –
Zhang et al. 2024 – – – – -0.372* – – –
Hunt & Reffert 2024 – – – – – 538* – –
Cavallo et al. 2024 4.17 2.14 – 1148 -0.250 – – –
Hunt & Reffert 2023 4.54 2.13 1.32 851 – – – –

(*): Indicates that this parameter is assigned more than one value in the corresponding reference.

Visualization

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